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SUMMARY:A view of the cosmic web through the lens of HI galaxies - Madalin
 a Tudorache (IoA)
DTSTART:20251212T113000Z
DTEND:20251212T123000Z
UID:TALK236068@talks.cam.ac.uk
CONTACT:Sandro Tacchella
DESCRIPTION:Galaxies do not form in isolation\, they grow within the large
  scale filaments\, which affect their formation and evolution. However\, t
 he extent to which the filaments shape galaxies has not been yet understoo
 d. Particularly\, how the proximity to filaments affects the ability of ga
 laxies to accrete gas to sustain their star formation. Moreover\, the orie
 ntation of a galaxy with respect to the filament can provide important ins
 ights into its intrinsic properties. In this talk\, I will present the res
 ults from the state-of-art radio survey MIGHTEE-HI conducted with the Meer
 KAT radio telescope (an SKA pathfinder) and show how observations of neutr
 al hydrogen in galaxies are instrumental to enhance our knowledge of galax
 ies growth\, as well as shed the light on the star formation histories (SF
 Hs) of spiral galaxies in relation to their large scale environment.\n
LOCATION:Ryle Seminar Room\, KICC + online
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